Results 171 to 180 of about 16,853 (286)
Convective Overstability in Radially Global Protoplanetary Disks. I. Pure Gas Dynamics
Protoplanetary disks are prone to several hydrodynamic instabilities. One candidate, convective overstability (COS), can drive radial semiconvection that may influence dust dynamics and planetesimal formation.
Marius Lehmann, Min-Kai Lin
doaj +1 more source
Organic Matter in the Asteroid Ryugu: What We Know So Far. [PDF]
Potiszil C+8 more
europepmc +1 more source
Linking asteroids and meteorites to the primordial planetesimal population
R. Greenwood, T. Burbine, I. Franchi
semanticscholar +1 more source
Impact processing of chondritic planetesimals: Siderophile and volatile element fractionation in the Chico L chondrite [PDF]
M. D. Norman, David W. Mittlefehldt
openalex +1 more source
Dynamical Evolution of Planetesimals in Protoplanetary Disks [PDF]
Roman R. Rafikov
openalex +1 more source
Imaging of the Vega Debris System Using JWST/MIRI
We present images of the Vega planetary debris disk obtained at 15.5, 23, and 25.5 μ m with the Mid-Infrared Instrument on JWST. The debris system is remarkably symmetric, smooth, and centered accurately on the star.
Kate Y. L. Su+8 more
doaj +1 more source
Possible Ribose Synthesis in Carbonaceous Planetesimals. [PDF]
Paschek K+7 more
europepmc +1 more source
PLANETARY MIGRATION IN EVOLVING PLANETESIMAL DISKS [PDF]
I. S. Yeşilyurt+2 more
openalex +1 more source
Particle Pileups and Planetesimal Formation [PDF]
Andrew N. Youdin, Eugene Chiang
openalex +1 more source
Distinguishing the Origin of Asteroid (16) Psyche. [PDF]
Elkins-Tanton LT+21 more
europepmc +1 more source